Detection of Compton Scattering in the Jet of 3C 84

3C 84 is the brightest cluster galaxy in the Perseus Cluster. It is among the closest radio-loud active galaxies and among the very few that can be detected from low-frequency radio up to TeV <em>γ</em>-rays. Here we report on the first X-ray polarization observation of 3C 84 with the Imaging X-ray Polarimetry Explorer, for a total of 2.2 Ms coinciding with a flare in <em>γ</em>-rays. This is the longest observation for a radio-loud active galaxy, which allowed us to reach unprecedented sensitivity, leading to the detection of an X-ray polarization degree of Π<sub>X</sub> = 4.2% ± 1.3% (∼3.2<em>σ</em> confidence) at an X-ray electric vector polarization angle of <em>ψ</em><sub>X</sub> = 163° ± 9°, which is aligned with the radio jet direction on the sky. Optical polarization observations show fast variability about the jet axis as well. Our results strongly favor models in which X-rays are produced by Compton scattering from relativistic electrons—specifically synchrotron self-Compton—that takes place downstream, away from the supermassive black hole.<br>

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Journal
SPIRE - Sciences Po Institutional REpository
Published
2025-11-11
DOI
https://doi.org/10.3847/2041-8213/ae157d
Primary Topic
Astrophysics and Cosmic Phenomena
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article
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article

Detection of Compton Scattering in the Jet of 3C 84

Fabian Kislat, Ildar Khabibullin, Laura Di Gesu, Thibault Barnouin et al.
SPIRE - Sciences Po Institutional REpository
Astrophysics and Cosmic Phenomena
article

Detection of Compton Scattering in the Jet of 3C 84

Fabian Kislat, Ildar Khabibullin, Laura Di Gesu, Thibault Barnouin, Dawoon E. Kim, A. A. Vasilyev, Daniel Morcuende, Chien‐Ting Chen, A. Sota, A. Kraus, Ioannis Liodakis, А. В. Жовтан, Pouya M. Kouch, Y. Y. Kovalev, E. Costa, Garrett K. Keating, F. Tavecchio, E. Angelakis, Diego Álvarez-Ortega, Sincheol Kang, M. Lynne Saade, P. Soffitta, A. Strigachev, T. Pursimo, Jorge Otero-Santos, Martin C. Weisskopf, Е. Г. Ларионова, Yu. V. Troitskaya, С. С. Савченко, V. Fallah Ramazanı, O. J. Roberts, I. Myserlis, T. S. Grishina, I. Agudo, Francesco Tombesi, Ramprasad Rao, Frédéric Marin, D. A. Morozova, Steven R. Ehlert, Sudip Chakraborty, Stephen L. O’Dell, Hyeon‐Woo Jeong, F. J. Aceituno, E. N. Kopatskaya, I. S. Troitskiy, Riccardo Ferrazzoli, Sang-Sung Lee, G. Bonnoli, Giorgio Galanti, E. Lindfors, V. Casanova, K. Nilsson, Г. А. Борман, Douglas A. Swartz, Chanwoo Song, Whee Yeon Cheong, Georgios Filippos Paraschos, C. Casadio, Jenni Jormanainen, R. Middei, E. Churazov, Mark Gurwell, L. Pacciani, Alan P. Marscher, P. Kaaret, Ajay Ratheesh, S. W. Li, Anna Trindade Falcão, R. Bachev, M. Roncadelli, V. Piirola, Sang-Hyun Kim, V. A. Hagen-Thorn, Juan Escudero, Myoung-Seok Nam, Jacob Casey, Gabriel Emery, Ekaterina V. Shishkina
article en

Abstract

3C 84 is the brightest cluster galaxy in the Perseus Cluster. It is among the closest radio-loud active galaxies and among the very few that can be detected from low-frequency radio up to TeV <em>γ</em>-rays. Here we report on the first X-ray polarization observation of 3C 84 with the Imaging X-ray Polarimetry Explorer, for a total of 2.2 Ms coinciding with a flare in <em>γ</em>-rays. This is the longest observation for a radio-loud active galaxy, which allowed us to reach unprecedented sensitivity, leading to the detection of an X-ray polarization degree of Π<sub>X</sub> = 4.2% ± 1.3% (∼3.2<em>σ</em> confidence) at an X-ray electric vector polarization angle of <em>ψ</em><sub>X</sub> = 163° ± 9°, which is aligned with the radio jet direction on the sky. Optical polarization observations show fast variability about the jet axis as well. Our results strongly favor models in which X-rays are produced by Compton scattering from relativistic electrons—specifically synchrotron self-Compton—that takes place downstream, away from the supermassive black hole.<br>

SPIRE - Sciences Po Institutional REpository
Boston University (US), University of Rome Tor Vergata (IT), Physical Research Laboratory (IN), Marshall Space Flight Center (US), Centre National de la Recherche Scientifique (FR), Goddard Space Flight Center (US), Universities Space Research Association (US), University of Crete (GR), University of Turku (FI), Istituto Nazionale di Fisica Nucleare (IT), University of New Hampshire (US), St Petersburg University (RU), National and Kapodistrian University of Athens (GR), Aarhus University (DK), Astronomical Observatory of Rome (IT), Agenzia Spaziale Italiana (IT), Korea Astronomy and Space Science Institute (KR), Pulkovo Observatory (RU), Observatoire astronomique de Strasbourg (FR), Brera Astronomical Observatory (IT), University of Chicago (US), Institute for Space Astrophysics and Planetology (IT), Max Planck Institute for Astrophysics (DE), Istituto Nazionale di Fisica Nucleare, Sezione di Padova (IT), Istituto di Astrofisica Spaziale e Fisica Cosmica di Milano (IT), Istituto Nazionale di Fisica Nucleare, Sezione di Pavia (IT), Istituto Nazionale di Fisica Nucleare, Roma Tor Vergata (IT), Institute of Astronomy and National Astronomical Observatory (BG), Center for Astrophysics Harvard & Smithsonian (US), Nordic Optical Telescope (ES), Instituto de Radioastronomía Milimétrica (ES), Max Planck Institute for Radio Astronomy (DE), Instituto de Astrofísica de Andalucía (ES), Crimean Astrophysical Observatory (UA), Université de Strasbourg (FR), Ludwig-Maximilians-Universität München (DE), Korea University of Science and Technology (KR), Foundation for Research and Technology Hellas (GR), Aalto University (FI)
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Astrophysics and Cosmic Phenomena
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